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Interstellar extinction in the UV
Abstract
The UV interstellar extinction obtained from observations using the OAO-2, Copernicus and TD-1 satellites, is fitted to simple analytical expressions in the variable x = 1/λ. The feature centred at |$\lambda \simeq 2200$| Å can be fitted to a Lorentz profile; this result may be of physical significance.
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Cited by
The physical properties of star-forming galaxies in the low-redshift Universe
Brinchmann, J., Charlot, S., White, S. D. M., Tremonti, C., Kauffmann, G., Heckman, T., & Brinkmann, J. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07881.x · Cited by 3,290
Correcting for the Effects of Interstellar Extinction
Fitzpatrick, E. L. (1999) · Publications of the Astronomical Society of the Pacific · doi:10.1086/316293 · Cited by 3,220
Interstellar Dust and Extinction
Mathis, J. S. (1990) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.28.090190.000345 · Cited by 1,311
3D Ly α radiation transfer: I. Understanding Ly α line profile morphologies
Verhamme, A., Schaerer, D., & Maselli, A. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20065554 · Cited by 499
THE DUST ATTENUATION LAW IN DISTANT GALAXIES: EVIDENCE FOR VARIATION WITH SPECTRAL TYPE
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Metadata
- Authors
- Seaton, M. J.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1979-05-01
- Volume
- 187
- Issue
- 1
- Pages
- 73P-76P
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2004645596
- Cited by
- 984
- References
- 0
- FWCI
- 14.23
- Type
- journal article
- Language
- en
- Open access
- closed
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